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Scientific paper - Original scientific paper
Extended Higgs Sectors in Radiative Neutrino Models
Physics Letters B, 768 (2017); 330-336. https://doi.org/10.1016/j.physletb.2017.03.013
Antipin, Oleg; Čuljak, Petar; Kumerički, Krešimir; Picek, Ivica

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Antipin, O., Čuljak, P., Kumerički, K. & Picek, I. (2017). Extended Higgs Sectors in Radiative Neutrino Models. Physics Letters B, 768., 330-336. doi: 10.1016/j.physletb.2017.03.013

Antipin, Oleg, et al. "Extended Higgs Sectors in Radiative Neutrino Models." Physics Letters B, vol. 768, 2017, pp. 330-336. https://doi.org/10.1016/j.physletb.2017.03.013

Antipin, Oleg, Petar Čuljak, Krešimir Kumerički and Ivica Picek. "Extended Higgs Sectors in Radiative Neutrino Models." Physics Letters B 768 (2017): 330-336. https://doi.org/10.1016/j.physletb.2017.03.013

Antipin, O., et al. (2017) 'Extended Higgs Sectors in Radiative Neutrino Models', Physics Letters B, 768, pp. 330-336. doi: 10.1016/j.physletb.2017.03.013

Antipin O, Čuljak P, Kumerički K, Picek I. Extended Higgs Sectors in Radiative Neutrino Models. Physics Letters B [Internet]. 2017 [cited 2024 July 15];768:330-336. doi: 10.1016/j.physletb.2017.03.013

O. Antipin, P. Čuljak, K. Kumerički and I. Picek, "Extended Higgs Sectors in Radiative Neutrino Models", Physics Letters B, vol. 768, pp. 330-336, 2017. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:786595. [Accessed: 15 July 2024]

Metadata
Title (english)Extended Higgs Sectors in Radiative Neutrino Models
AuthorOleg Antipin
MBZ: 350622
AuthorPetar Čuljak
AuthorKrešimir Kumerički
MBZ: 194553
AuthorIvica Picek
MBZ: 74074
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
Testable Higgs partners may be sought within the extensions of the SM Higgs sector aimed at generating neutrino masses at the loop level. We study a viability of extended Higgs sectors for two selected models of radiative neutrino masses: a one-loop mass model, providing the Higgs partner within a real triplet scalar representation, and a three-loop mass model, providing it within its two- Higgs-doublet sector. The Higgs sector in the one- loop model may remain stable and perturbative up to the Planck scale, whereas the three-loop model calls for a UV completion around 106 GeV. Additional vector-like lepton and exotic scalar fields, which are required to close one- and three- loop neutrino-mass diagrams, play a decisive role for the testability of the respective models. We constrain the parameter space of these models using LHC bounds on diboson resonances.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titlePhysics Letters B
Numberingvol. 768, pp. 330-336
p-ISSN0370-2693
DOIhttps://doi.org/10.1016/j.physletb.2017.03.013
URN:NBNurn:nbn:hr:217:786595
Publication2017
ProjectNumber: IP-2013-11-8799
Title (croatian): Tvar i međudjelovanja na ubrzivačima i u svemiru
Acronym: MIAU
Leader: Krešimir Kumerički
Jurisdiction: Croatia
Funding stream: IP
Document URLhttps://www.sciencedirect.com/science/article/pii/S0370269317301910
Type of resourceText
Access conditionsOpen access
Terms of useLicence Attribution 4.0 International (CC BY 4.0) icon
Public note© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3. Published 10 May 2017.
Created on2020-02-28 20:42:58